The case for a 'sub-millimeter SDSS': a 3D map of galaxy evolution to z~10
by James Geach, Manda Banerji, Frank Bertoldi, Matthieu Bethermin, Caitlin M. Casey, Chian-Chou Chen, David L. Clements, Claudia Cicone, Francoise Combes, Christopher Conselice, Asantha Cooray, Kristen Coppin, Emanuele Daddi, Helmut Dannerbauer, Romeel Dave, Matthew Doherty, James S. Dunlop, Alastair Edge, Duncan Farrah, Maximilien Franco, Gary Fuller, Tracy Garratt, Walter Gear, Thomas R. Greve, Evanthia Hatziminaoglou, Christopher C. Hayward, Rob J. Ivison, Ryohei Kawabe, Pamela Klaassen, Kirsten K. Knudsen, Kotaro Kohno, Maciej Koprowski, Claudia D. P. Lagos, Georgios E. Magdis, Benjamin Magnelli, Sean L. McGee, Michal Michalowski, Tony Mroczkowski, Omid Noroozian, Desika Narayanan, Seb Oliver, Dominik Riechers, Wiphu Rujopakarn, Douglas Scott, Stephen Serjeant, Matthew W. L. Smith, Mark Swinbank, Yoichi Tamura, Paul van der Werf, Eelco van Kampen, Aprajita Verma, Joaquin Vieira, Jeff Wagg, Fabian Walter, Lingyu Wang, Al Wootten, and Min S. Yun
Published onMay 31, 2019
The case for a 'sub-millimeter SDSS': a 3D map of galaxy evolution to z~10
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Abstract
We argue that a 'sub-millimeter SDSS' - a sensitive large-area imaging+spectroscopic survey in the sub-mm window - will revolutionize our understanding of galaxy evolution in the early Universe.
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